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Churning galaxy is a snake pit

6 October 2011

Turbulence revealed: the 'snakes' are regions of gas where the density and magnetic field are changing rapidly as a result of turbulence. The image shows the gradient of linear polarisation over an 18-square-degree region of the Southern Galactic Plane. [Image: Bryan Gaensler et al. Data: CSIRO/ATCA]

A pit of writhing snakes—that's what the first picture of turbulent gas in our Milky Way looks like. Professor Bryan Gaensler of the University of Sydney and his team used a CSIRO radio telescope in eastern Australia to make the groundbreaking image, published in Nature today.

The space between the stars in our galaxy is not empty, but is filled with thin gas that continually swirls and churns.

Turbulence makes the universe magnetic, helps stars form, and spreads the heat from supernova explosions through the galaxy.

"We now plan to study turbulence throughout the Milky Way. Ultimately this will help us understand why some parts of the galaxy are hotter than others, and why stars form at particular times in particular places," Professor Gaensler said.

Gaensler and his team studied a region of our galaxy about 10,000 light-years away in the constellation Norma. They used CSIRO's Australia Telescope Compact Array because "it is one of the world's best telescopes for this kind of work," as Dr Robert Braun, Chief Scientist at CSIRO Astronomy and Space Science explained.

The radio telescope was tuned to receive radio waves that come from the Milky Way. As these waves travel through the swirling interstellar gas, one of their properties—polarisation—is very slightly altered, and the radio telescope can detect this. Polarisation is the direction the waves 'vibrate'. Light can be polarised: some sunglasses filter out light polarised in one direction while letting through other light.

The researchers measured the polarisation changes over an area of sky and used them to make a spectacular image of overlapping entangled tendrils, resembling writhing snakes. The 'snakes' are regions of gas where the density and magnetic field are changing rapidly as a result of turbulence.

The 'snakes' also show how fast the gas is churning—an important number for describing the turbulence. Team member Blakesley Burkhart, a PhD student from the University of Wisconsin, made several computer simulations of turbulent gas moving at different speeds.

These simulations resembled the 'snakes' picture, with some matching the real picture better than others. By picking the best match, the team concluded that the speed of the swirling in the turbulent interstellar gas is around 70,000 kph—relatively slow by cosmic standards.